PPT-Nearby Galaxy Evolution

Prof Gerhardt R Meurer Galaxy evolution in a nutshell Galaxy Evolution 2 Time machines The farther we peer The farther back in time we see Reveal cosmic history Hubble to lt 1 Gyr after big bang. Formation and cosmic evolution of massive black holes. Andrea Merloni. MPE, Garching. Syllabus. Monday:. Observational evidence of Supermassive Black Holes. AGN surveys. Tuesday: . The evolution of SMBH mass function and spin distributions. Low-. Redshift. Galaxies. Adam Leroy (NRAO, North American ALMA Science Center). HERACLES & THINGS teams: . Fabian Walter, Andreas . Schruba. , Frank . Bigiel. , Elias Brinks, Erwin . de . Blok, Kelly . は階層的銀河形成論で説明. できるか？. Motohiro. 　. Enoki. Tomoaki Ishiyama (Tsukuba Univ.). Masakazu A. R. Kobayashi (Ehime Univ.). Masahiro . Nagashima. . (Nagasaki Univ. .). §1. Introduction. a prospect from galaxy evolution. Cosmic Microwave Background Radiation and Its Foreground Interstellar Components, Tokyo. , . 17. th. February, 2010. Tsutomu T. TAKEUCHI. Institute for Advanced Research, Nagoya University, Japan. Life in the Universe. Chapter 18. Life in the Universe. Units of Chapter 18. Cosmic Evolution. Life in the Solar System. Intelligent Life in the Galaxy. The Search for Extraterrestrial . Intelligence. galaxy group, Stephan D. Calzetti (Univ. of Massachusetts). a. nd the LEGUS . Team. https://. legus.stsci.edu. /. HUBBLE2020: Hubble’s 25. th. Anniversary Symposium. STScI. , Baltimore, April 20-24, 2015. NGC3344. NGC1566. around Abell 370, . a galaxy cluster at z = 0.37. International SKA . Forum 2010 . Philip Lah. A New Golden Age for Radio Astronomy. Collaborators:. . Frank Briggs (ANU). . Michael Pracy . Here’s the Story We’ll Unfold for You…. Hubble’s galaxy classifications: Spirals, . ellipticals. , irregulars. . Structural parts of galaxies: disk, halo, nucleus, bulge. Spiral arms – tracers of star formation. Here’s the Story We’ll Unfold for You…. Hubble’s galaxy classifications: Spirals, . ellipticals. , irregulars. . Structural parts of galaxies: disk, halo, nucleus, bulge. Spiral arms – tracers of star formation. M82 – Cigar Galaxy. ASTR 2401. Goal. Target selection. Object information. Data collection. Image calibration. Processing. Mosaicing. Perils of Astrophotography. Final image. References. Goal. To capture color images of an object or objects that required mosaic work to form the final image. . Here’s the Story We’ll Unfold for You…. Hubble’s galaxy classifications: Spirals, . ellipticals. , irregulars. . Structural parts of galaxies: disk, halo, nucleus, bulge. Spiral arms – tracers of star formation. Laura . Magrini. INAF- . Osservatorio. . Astrofisico. di . Arcetri. In Our Galaxy. Open clusters (disc population): . Many (~2200 known clusters). . even more new candidates in the inner disc from infrared surveys . Where we are and . where we are going.. D.J. Pisano . (WVU). djpisano@mail.wvu.edu. The Big Questions . How does the gas content of galaxies evolve over cosmic time and in different environments?. How does gas flow into and out of galaxies?.